Multiplicity (statistical mechanics) explained
In statistical mechanics, multiplicity (also called statistical weight) refers to the number of microstates corresponding to a particular macrostate of a thermodynamic system.[1] Commonly denoted
, it is related to the
configuration entropy of an isolated system
[2] via
Boltzmann's entropy formulawhere
is the
entropy and
is the
Boltzmann constant.
Example: the two-state paramagnet
A simplified model of the two-state paramagnet provides an example of the process of calculating the multiplicity of particular macrostate.[1] This model consists of a system of microscopic dipoles which may either be aligned or anti-aligned with an externally applied magnetic field . Let
represent the number of dipoles that are aligned with the external field and
represent the number of anti-aligned dipoles. The energy of a single aligned dipole is
while the energy of an anti-aligned dipole is
thus the overall energy of the system is
The goal is to determine the multiplicity as a function of ; from there, the entropy and other thermodynamic properties of the system can be determined. However, it is useful as an intermediate step to calculate multiplicity as a function of
and
This approach shows that the number of available macrostates is . For example, in a very small system with dipoles, there are three macrostates, corresponding to
Since the
and
macrostates require both dipoles to be either anti-aligned or aligned, respectively, the multiplicity of either of these states is 1. However, in the
either dipole can be chosen for the aligned dipole, so the multiplicity is 2. In the general case, the multiplicity of a state, or the number of microstates, with
aligned dipoles follows from
combinatorics, resulting in
where the second step follows from the fact that
Since
N\uparrow-N\downarrow=-\tfrac{U}{\muB},
the energy can be related to
and
as follows:
Thus the final expression for multiplicity as a function of internal energy is
This can be used to calculate entropy in accordance with Boltzmann's entropy formula; from there one can calculate other useful properties such as temperature and heat capacity.
Notes and References
- Book: Schroeder . Daniel V. . An Introduction to Thermal Physics . 1999 . Pearson . 9780201380279 . First.
- Book: Atkins, Peter. Julio de Paula. 2002. Physical Chemistry. 7th. Oxford University Press.